MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil

Abstract Right-handed neutrinos with MeV to GeV mass are very promising candidates for dark matter (DM). Not only can they solve the missing satellite puzzle, the cusp-core problem of inner DM density profiles, and the too-big-to fail problem, i.e. that the unobserved satellites are too big to not h...

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Main Authors: Juri Fiaschi, Michael Klasen, Miguel Vargas, Christian Weinheimer, Sybrand Zeinstra
Format: Article
Language:English
Published: SpringerOpen 2019-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP11(2019)129
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spelling doaj-e280bcf8b84e4325866f8900b00f4b692020-11-25T04:11:56ZengSpringerOpenJournal of High Energy Physics1029-84792019-11-0120191112610.1007/JHEP11(2019)129MeV neutrino dark matter: relic density, lepton flavour violation and electron recoilJuri Fiaschi0Michael Klasen1Miguel Vargas2Christian Weinheimer3Sybrand Zeinstra4Institut für Theoretische Physik, Westfälische Wilhelms-Universität MünsterInstitut für Theoretische Physik, Westfälische Wilhelms-Universität MünsterInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitut für Kernphysik, Westfälische Wilhelms-Universität MünsterInstitut für Theoretische Physik, Westfälische Wilhelms-Universität MünsterAbstract Right-handed neutrinos with MeV to GeV mass are very promising candidates for dark matter (DM). Not only can they solve the missing satellite puzzle, the cusp-core problem of inner DM density profiles, and the too-big-to fail problem, i.e. that the unobserved satellites are too big to not have visible stars, but they can also account for the Standard Model (SM) neutrino masses at one loop. We perform a comprehensive study of the right-handed neutrino parameter space and impose the correct observed relic density and SM neutrino mass differences and mixings. We find that the DM masses are in agreement with bounds from big-bang nucleosynthesis, but that these constraints induce sizeable DM couplings to the charged SM leptons. We then point out that previously overlooked limits from current and future lepton flavour violation experiments such as MEG and SINDRUM heavily constrain the allowed parameter space. Since the DM is leptophilic, we also investigate electron recoil as a possible direct detection signal, in particular in the XENON1T experiment. We find that despite the large coupling and low backgrounds, the energy thresholds are still too high and the predicted cross sections too low due to the heavy charged mediator, whose mass is constrained by LEP limits.http://link.springer.com/article/10.1007/JHEP11(2019)129Beyond Standard ModelCosmology of Theories beyond the SMNeutrino Physics
collection DOAJ
language English
format Article
sources DOAJ
author Juri Fiaschi
Michael Klasen
Miguel Vargas
Christian Weinheimer
Sybrand Zeinstra
spellingShingle Juri Fiaschi
Michael Klasen
Miguel Vargas
Christian Weinheimer
Sybrand Zeinstra
MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
Neutrino Physics
author_facet Juri Fiaschi
Michael Klasen
Miguel Vargas
Christian Weinheimer
Sybrand Zeinstra
author_sort Juri Fiaschi
title MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil
title_short MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil
title_full MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil
title_fullStr MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil
title_full_unstemmed MeV neutrino dark matter: relic density, lepton flavour violation and electron recoil
title_sort mev neutrino dark matter: relic density, lepton flavour violation and electron recoil
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2019-11-01
description Abstract Right-handed neutrinos with MeV to GeV mass are very promising candidates for dark matter (DM). Not only can they solve the missing satellite puzzle, the cusp-core problem of inner DM density profiles, and the too-big-to fail problem, i.e. that the unobserved satellites are too big to not have visible stars, but they can also account for the Standard Model (SM) neutrino masses at one loop. We perform a comprehensive study of the right-handed neutrino parameter space and impose the correct observed relic density and SM neutrino mass differences and mixings. We find that the DM masses are in agreement with bounds from big-bang nucleosynthesis, but that these constraints induce sizeable DM couplings to the charged SM leptons. We then point out that previously overlooked limits from current and future lepton flavour violation experiments such as MEG and SINDRUM heavily constrain the allowed parameter space. Since the DM is leptophilic, we also investigate electron recoil as a possible direct detection signal, in particular in the XENON1T experiment. We find that despite the large coupling and low backgrounds, the energy thresholds are still too high and the predicted cross sections too low due to the heavy charged mediator, whose mass is constrained by LEP limits.
topic Beyond Standard Model
Cosmology of Theories beyond the SM
Neutrino Physics
url http://link.springer.com/article/10.1007/JHEP11(2019)129
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